Solar Radiation Physical Modeling (SRPMv2)
and the Sun-Earth Radiative Connection
Supported by: J.M. Fontenla
firstname.lastname@example.org or email@example.com
First Version: 2001/2/2
Current Version: 2010/10/15
Site still under development, some links may not work...The SRPM current data includes a set of physical models for the main features responsible for the solar radiative output and its variations with the solar cycle.
Photospheric-chromospheric temperature, and height, as function of pressure in the current set of models.
Charged particles (ne, np, and nion=sum(n_i)) and neutral hydrogen (na) densities as function of pressure in the current set of models.
Plasma parameters: Mean ion mass, m_ion=sum(n_i*m_i)/nion, in units of the hydrogen mass, and Ion acoustic velocity, sqrt(2*k*T/m_ion).